Station
Similar stations in BD-02 4304
Surface Port - 109 Ls
Democrats of BD-02 4304
Bean Enterprise
Starport (Coriolis) - 139 Ls
Social Eleu Progressive Party
Simak Town
Surface Port - 142 Ls
Democrats of BD-02 4304
Gell-Mann Dock
Starport (Coriolis) - 153 Ls
Social Eleu Progressive Party
Durrance Station
Starport (Coriolis) - 287 Ls
BD-02 4304 Gold Major Holdings
Tanner Installation
Surface Port - 890 Ls
Social Eleu Progressive Party
Brandenstein Enterprise
Outpost (Civilian) - 901 Ls
BD-02 4304 Gold Major Holdings
Abbott Arsenal
Surface Port - 5,464 Ls
Social Eleu Progressive Party
Currie Terminal
Outpost (Civilian) - 5,835 Ls
Social Eleu Progressive Party
Fabian Dock
Outpost (Civilian) - 5,943 Ls
Democrats of BD-02 4304
Newton Dock
Starport (Orbis) - 5,963 Ls
Social Eleu Progressive Party
Galpedia
Eugene Parker
Eugene N. Parker (born June 10, 1927) is an American solar astrophysicist who received his B.S. degree in physics from Michigan State University in 1948 and Ph.D. from Caltech in 1951. In the mid-1950s Parker developed the theory on the supersonic solar wind and predicted the Parker spiral shape of the solar magnetic field in the outer solar system. In 1987, Parker proposed that the solar corona might be heated by myriad tiny "nanoflares", miniature brightenings resembling solar flares that would occur all over the surface of the Sun.
Parker was elected to the National Academy of Sciences in 1967. As of early 2005, he was still engaged in active research at the University of Chicago. His daughter and son-in-law are both faculty members at Michigan State University.
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